Alpha Arae, is the second brightest star in the southern constellation of Ara. Its name is a Bayer designation that is Latinized from α Arae, and abbreviated Alpha Ara or α Ara. With an average apparent visual magnitude 2.93,[ it is readily visible to the naked eye from the southern hemisphere. This star is close enough to the Earth that its distance can be estimated using stellar parallax data collected during the Hipparcos mission. It is around away, with a 7% margin of error. The visual magnitude of the star is diminished by 0.10 magnitudes as a result of extinction from intervening gas and dust.][
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Properties
Alpha Arae has a stellar classification of B2 Vne,[ indicating that it is a massive B-type main sequence star. The 'n' notation in the suffix indicates that the in the star's stellar spectrum appear spread out and nebulous because of the Doppler effect from rapid rotation. The measured projected rotational velocity has been measured as high as .][ Meilland et al. (2007) estimate the pole of the star is inclined by 55° to the line of sight, yielding an equatorial velocity of . This is close to the critical velocity where the star would start to break up.][ The rapid rotation is causing a pronounced equatorial bulge of about 2.4–2.7 times the polar radius.][
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It is a Be star, as indicated by the 'e' notation in the star's classification. This indicates that are observed in the spectrum, which is coming from a disk of material ejected from the star because of its rapid rotation.[ In 2003 and 2005, Alpha Arae was observed by infrared interferometry, using the MIDI and AMBER instruments at the VLT Interferometer. The results, published in 2005 and 2007, appear to show that Alpha Arae is surrounded by a dense equatorial disk of material in Keplerian (rather than uniform) rotation, and that it is losing mass by a polar stellar wind with a terminal velocity of approximately 1,000 km/s. There is also some evidence that Alpha Arae is orbited by a companion at 0.7 AU.][
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This star is around 9.6 times as massive as the Sun,[ It is 5,800 times as luminous as the Sun,][ This heat gives Alpha Arae the blue-white hue that is characteristic of . It is a variable star with a magnitude that varies between 2.76m and 2.90m.][ The International Variable Star Index defines it as GCAS + LERI, showing both rapid periodic variation and slow irregular eruptions.][
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Alpha Arae has a double star, CCDM J17318-4953B, located approximately 50 away along a position angle of 168°, with an apparent visual magnitude of about 11.[ The two stars appear close to each other by coincidence and are not physically close in space.]
In culture
With Beta Arae and Sigma Arae it forms the Chinese asterism Choo (pinyin: chǔ, 杵), "pestle" in traditional Chinese astronomy. It was the second star of Choo (杵二), but R. H. Allen used the name Choo for this star only.[ This name is also given the French spelling Tchou. There is another Choo in the constellation Pegasus.
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In Chinese, 杵 (Chǔ), meaning Pestle, refers to an asterism consisting of α Arae, Sigma Arae and Beta Arae.[ 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, .] Consequently, the Chinese name for α Arae itself is 杵二 (Chǔ èr, ).[ 香港太空館 - 研究資源 - 亮星中英對照表 , Hong Kong Space Museum. Accessed on line November 23, 2010.]
See also
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Traditional Chinese star names in Ara
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Traditional Chinese star names in Pegasus
[ See Tables 1 and 4 for parameters of the star, circumstellar disk, and polar winds.]
[ CDS ID V/50. Accessed on line November 26, 2008.]
External links
